 I. All self-luminous bodies in the celestial spaces are composed of meteorites, or masses of meteoritic vapour produced by heat brought about by condensation of meteor-swarms due to gravity. II. The spectra of all bodies depend upon the heat of the meteorites,...  Advanced Physiography - Page 300by John Thornton (M.A.) - 1890 - 342 pagesFull view - About this book
 | Royal Society (Great Britain) - Electronic journals - 1888 - 624 pages
...by heat brought about by condensation of meteor-swarms due to gravity. II. The spectra of all such bodies depend upon the heat of the meteorites, produced...temperature of the vapours produced by collisions in nebulee, stars without C and F but with other bright lines, and in comets away from perihelion, is... | |
 | Sir Norman Lockyer - Electronic journals - 1888 - 668 pages
...produced by heat brought about by condensation of meteor-swarms due to gravity. II. The spectra of nil bodies depend upon the heat of the meteorites, produced...swarms upon the time which has elapsed since complete vaporization. III. The temperature of the vapours produced by collisions in nebula;, stars without... | |
 | Astronomy - 1887 - 470 pages
...meteorites, or masses of meteoritic vapour produced by heat brought about by condensation of meteor-swarms due to gravity. " II. The spectra of all bodies depend...swarms, upon the time which has elapsed since complete vaporization " VII. The existing distinction between stars, comets, and nebulae rests on no physical... | |
 | Royal Society (Great Britain) - Science - 1888 - 586 pages
...condensation of meteor-swarms due to gravity. II. The spectra of all such bodies depend upon the heat of t'le meteorites, produced by collisions, and the average...stars without C and F but with other bright lines, and ili comets away from perihelion, is about that of the bunsen burner. IV. The temperature of the vapours... | |
 | Sir Norman Lockyer - Electronic journals - 1888 - 900 pages
...meteorites, or masses of meteoritic vapour produced by heat brought about by condensation of meteor-swarms due to gravity. II. The spectra of all bodies depend...swarms upon the time which has elapsed since complete vaporization. III. The temperature of the vapours produced by collisions in nebulx, stars without C... | |
 | Sir Norman Lockyer - Electronic journals - 1888 - 674 pages
...meteorites, or masses of meteoritic vapour produced by heat brought about by condensation of meteor-swarms due to gravity. II. The spectra of all bodies depend...swarms upon the time which has elapsed since complete vaporization. III. The temperature of the vapours produced by collisions in nebula:, stars without... | |
 | Science - 1888 - 868 pages
...meteorites, or masses of meteoritic vapour produced by heat brought about by condensation of meteor-swarms due to gravity. II. The spectra of all bodies depend...swarms upon the time which has elapsed since complete vaporization. III. The temperature of the vapours produced by collisions in nebula:, stars without... | |
 | Science - 1888 - 920 pages
...meteoric vapor, produced by heat brought about by condensation of meteor swarms due to gravity ; that the spectra of all bodies depend upon the heat of...and the average space between the meteorites in the ewarm, or in the cose of consolidated swarms, upon the time which has elapsed since complete vaporization... | |
 | George Frederick Chambers - Astronomical instruments - 1890 - 602 pages
...by heat brought about by condensation of meteor-fwarms due to gravity. " (2) The spectra of all such bodies depend upon the heat of the meteorites, produced...time which has elapsed since complete vaporisation " (7) The existing distinction between stars, comets, and nebulee rests on no physical basis. " (8)... | |
 | Sir Norman Lockyer - Meteoritic hypothesis - 1890 - 600 pages
...as comets do on Schiaparelli's hypothesis. 4. The spectra of all cosmical bodies depend upon either the heat of the meteorites produced by collisions,...between the meteorites in the swarm ; or, in the case of swarms wholly volatilised, upon the loss by radiation since complete vaporisation. 5. The temperature... | |
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